Refractory metals such as Ti, Zr, Hf, V, Nb, and Ta can dissolve oxygen up to 33 %, 29 %, 20 %, 17 %, 9 %, and 5.7 %, respectively, at high temperatures. The high solubility of oxygen causes brittleness in these metals. When designing a refractory high entropy alloy, efforts should be focused on reducing oxygen solubility. We find that the high solubility of oxygen is related to the thermodynamic stability of oxygen interstitials in pure refractory metals. To understand the impact of alloy composition on oxygen solubility in refractory alloys, we examine the thermodynamic stability of oxygen interstitials across various refractory binary alloys. Using first-principles Density Functional Theory (DFT), we calculate the Oxygen Interstitial Formation Energy (OIFE) of nine refractory metals and their 24 equiatomic binary alloys. The OIFE is determined by the bond strength between oxygen and the nearest neighbor (NN) metal atoms. It is a strong function of the nature of NN atoms that surround the interstitial site rather than the overall composition of the alloy. For a given alloy, the OIFE can vary based on the NN atoms around the oxygen interstitial. These observations indicate that an alloy with even a small amount of metal of high oxygen affinity (or highly negative OIFE), like Ti, can result in the high stability of oxygen in specific interstitial sites where the nearest neighbors are predominantly Ti atoms. It also explains Re as a choice of alloying elements to ductilize W instead of Ti. Although both Ti and Re alloying in W similarly improve its ductility, Ti’s tendency to stabilize oxygen interstitials makes the W-Ti alloy brittle, while Re does not stabilize oxygen interstitials.
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